Stability Of Planetary Orbits

Stability of Planetary Orbits is a theoretical construct in celestial mechanics that characterizes the long-term persistence of planetary trajectories within bounded deviations from nominal paths under perturbative gravitational influences.

341

Publications

23K

Citations

729

Authors

307

Institutions

Publications per year

2017–2026

53

Authors

729

  1. RD
    R. Dvořák

    University of Vienna, Austria

    16 publications · 788 citations

    15

    h-index

  2. JJ
    Jack J. Lissauer

    Ames Research Center, United States

    14 publications · 1.7K citations

    13

    h-index

  3. RB
    Rory Barnes

    University of Washington, United States

    9 publications · 579 citations

    10

    h-index

  4. JH
    Jonathan Horner

    UNSW Sydney, Australia

    9 publications · 472 citations

    9

    h-index

  5. MC
    M. Cuntz

    The University of Texas at Arlington, United States

    9 publications · 450 citations

    9

    h-index

1–5 of 729

Venues

  1. The Astrophysical Journal

    ApJ · 56 publications · 6.4K citations

    45

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    51 publications · 2.1K citations

    29

    h-index

  3. The Astronomical Journal

    AJ · 37 publications · 3.7K citations

    27

    h-index

  4. Astronomy and Astrophysics

    31 publications · 1.3K citations

    22

    h-index

  5. Celestial Mechanics and Dynamical Astronomy

    26 publications · 946 citations

    18

    h-index

1–5